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An Introduction to Mean Field Dynamo Theory
Chapter 2 An Introduction to Mean Field Dynamo Theory D.W. Hughes and S.M. Tobias Department of Applied Mathematics, University of Leeds 2.1 Introduction Magnetic fields are essentially ubiquitous, being detected over a tremen dous range of scales in planets, stars, accretion discs and in the interstellar medium. The dynamic behaviour of such fields is then responsible for a vast range of astrophysical phenomena (see, for example, Parker 1979). For instance, the solar magnetic field gives rise to sunspots, solar flares and coronal mass ejections; it also plays a major role in shaping the solar wind which, on interacting with the Earth's magnetic field, causes auro rae. Starspots, analogous to sunspots but covering a much greater surface area, have been detected on a number of cool stars. The pulsed emission of pulsars is a consequence of an extremely strong magnetic field. On the largest scales, the interstellar magnetic field plays a role in star formation, mediating angular momentum transport as the star collapses. The ulti mate question in the 'study of astrophysical magnetic fields must then be that of the origin of the magnetic field in cosmical objects. In particu lar, one might ask whether the observed magnetic fields are simply 'fossil fields', or whether, alternatively, they are being continually regenerated - i.~. whether some sort of dynamo process is taking place. For collision-dominated plasmas with short mean free paths, such as those found in stellar interiors, the evolution of magnetic fields is very well described by the equations of single-fluid magnetohydrodynamics (MHD). 15 16 Relaxation Dynamics in Laboratory and Astrophysical Plasmas (Although, for example, in studies of stellar atmospheres - such as the solar corona - the use of MHD is not based on such solid foundations.) In this review we shall be concerned only with physical systems for which the MHD description is appropriate. -
Space Plasma Physics Thomas Wiegelmann, 2012 Space Plasma Physics
4/18/2012 Space Plasma Physics Thomas Wiegelmann, 2012 Space Plasma Physics 1. Basic Plasma Physics concepts 2. Overview about solar system plasmas Physical Processes Plasma Models 8. Plasma Waves, instabilities and shocks 9. Magnetic Reconnection 3. Single particle motion, Test particle model 4. Statistic description of plasma, BBGKY- Applications Hierarchy and kinetic equations 10. Planetary Magnetospheres 5. Fluid models, Magneto-Hydro-Dynamics 11. Solar activity 6. Magneto-Hydro-Statics 7. Stationary MHD and Sequences of Equilibria 12. Transport Processes in Plasmas Used Material What is plasma? • Lecture notes from Eckart Marsch 2007 In plasma physics we study ionized gases • Baumjohann&Treumann: Basic Space Plasma Physics under the influence of • Schindler: Physics of space plasma activity electro-magnetic fields. • Priest: Solar MHD • Kulsrud: Plasma Physics for Astrophysics • Krall & Trivelpiece: Principles of Plasma Physics • Chen: Introduction to plasma physics and controlled fusion • Balescu: Plasma Transport (3 volumes) Levi Tonks (1897-1971) and William Crookes (1832-1919) • Spatschek: Theoretische Plasmaphysik Irving Langmuir (1881- called ionized matter in a gas 1957, photo) first used the discharge (Crookes-tube, photo) term plasma for a 4th state of matter • Wikipedia, Google and YouTube collection of charged (Phil. Trans 1879) particles (Phys. Rev. 1929) Source: Wikipedia Industrial Plasmas Natural Plasmas on Earth Lightning Electric Arcs St. E Fire Semi conducter Nuclear Fusion, Neon-lights, Fluorescent device fabrication lamps,Plasma globes here a Tokamak Ball lightning Aurorae Source: Wikipedia 1 4/18/2012 Space Plasmas Accretion discs Interior and atmosphere of Sun+Stars Source: Wikipedia Planetary magnetospheres, solar wind, inter-planetary medium Comparison: Gas and Plasma Source: Wikipedia Plasmas studied in this lecture What is a plasma? • Non-relativistic particle velocities v<<c • Spatial and temporal scales are large compared to • A fully or partly ionized gas. -
Space Plasma Physics
Space plasma physics • Basic plasma properties and equations • Space plasmas, examples and phenomenology • Single particle motion and trapped particles • Collisions and transport phenomena • Elements of kinetic theory • Fluid equations and magnetohydrodynamics • Magnetohydrodynamic waves Space plasma physics • Boundaries, shocks and discontinuities • Plasma waves in the fluid picture I • Plasma waves in the fluid picture II • Fundamentals of wave kinetic theory • Concepts of plasma micro- and macroinstability • Kinetic plasma microinstabilities • Wave-particle interactions 1 Basic plasma properties and equations • Definition of a plasma • Space plasmas - phenomenology • Parameters • Currents and charge densities • Composition and ionization • Maxwell‘s equations and forces • Induction equation Definition of a plasma A plasma is a mixed gas or fluid of neutral and charged particles. Partially or fully ionized space plasmas have usually the same total number of positive (ions) and negative (electrons) charges and therefore behave quasineutral. Space plasma particles are mostly free in the sense that their kinetic exceeds their potential energy, i.e. they are normally hot, T > 1000 K. Space plasmas have typically vast dimensions, such that the free paths of thermal particles are larger than the typical spatial scales --> they are collisionless. 2 Different types plasmas Plasmas differ by their chemical composition and the ionization degree of the ions or molecules (from different sources). Plasmas are mostly magnetized (internal and external